Results 11 to 20 of about 31,268 (166)
Energy exchange and wave action conservation for magnetohydrodynamic (MHD) waves in a general, slowly varying medium [PDF]
Annales Geophysicae, 2014 Magnetohydrodynamic (MHD) waves in the solar wind and magnetosphere are propagated in a medium whose velocity is comparable to or greater than the wave velocity and which varies in both space and time. In the approximation where the scales of the time
A. D. M. Walker
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Peculiarities of ULF wave characteristics in a multicomponent ionospheric plasma
Solar-Terrestrial Physics, 2022 We have examined the properties of low-frequency electromagnetic waves in multicomponent ionospheric plasma in the 1–30 Hz band, using the magnetoionic theory.
Kotik D. S. +2 more
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Mixed Properties of MHD Waves in Non-uniform Plasmas
Frontiers in Astronomy and Space Sciences, 2019 This paper investigates the mixed properties of MHD waves in a non-uniform plasma. It starts with a short revision of MHD waves in a uniform plasma of infinite extent. In that case the MHD waves do not have mixed properties.
Marcel L. Goossens +3 more
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Simulations of Incompressible MHD Turbulence [PDF]
, 2000 We simulate incompressible MHD turbulence in the presence of a strong background magnetic field. Our major conclusions are: 1) MHD turbulence is most conveniently described in terms of counter propagating shear Alfven and slow waves.
Goldreich, Peter, Maron, Jason
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Propagating MHD Waves in Coronal Holes [PDF]
Space Science Reviews, 2010 Coronal holes are the coolest and darkest regions of the solar atmosphere, as observed both on the solar disk and above the solar limb. Coronal holes are associated with rapidly expanding open magnetic fields and the acceleration of the high-speed solar wind.
Banerjee, D, Gupta, GR, Teriaca, L
openaire +3 more sources
Electromagnetic oscillations of the Earth's upper atmosphere (review) [PDF]
Annales Geophysicae, 2010 A complete theory of low-frequency MHD oscillations of the Earth's weakly ionized ionosphere is formulated. Peculiarities of excitation and propagation of electromagnetic acoustic-gravity, MHD and planetary waves are considered in the Earth's ...
A. G. Khantadze +5 more
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The Exact Solution of the Riemann Problem in Relativistic MHD [PDF]
, 2006 We discuss the procedure for the exact solution of the Riemann problem in special relativistic magnetohydrodynamics (MHD). We consider both initial states leading to a set of only three waves analogous to the ones in relativistic hydrodynamics, as well ...
Giacomazzo, B., Rezzolla, L.
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Linear and nonlinear resonant interaction of sound waves in dissipative layers [PDF]
, 2000 The theory of resonant nonlinear magnetohydrodynamic (MHD) waves in dissipative steady plasmas developed by Ballai and Erdélyi is used to study the effect of steady flows on nonlinear resonant heating of MHD waves in (a) linear, (b) weakly and (c ...
Ballai, I., Erdélyi, R., Goossens, M.
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Ducted compressional waves in the magnetosphere in the double-polytropic approximation [PDF]
Annales Geophysicae, 2002 Small-amplitude compressional magnetohydrodynamic-type waves are studied in the magnetosphere. The magnetosphere is treated as a rarefied plasma with anisotropy in the kinetic pressure distribution.
I. Ballai +4 more
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Cosmic ray fluctuations and MHD waves in the solar wind
Solar-Terrestrial Physics, 2023 During large-scale solar wind disturbances, variations in galactic cosmic rays with periods from several minutes to 2–3 hours, which are called cosmic ray fluctuations in the scientific literature, often occur.
Starodubtsev S. A. +3 more
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